We examined the size distributions of small L4 and L5 Jovian Trojan asteroids detected in the Subaru main belt asteroid survey (SMBAS). This was the first attempt to make a comparison of the size distribution between the L4 and L5 Trojans for sizes ranging from 1 km to 10 km, using the results of systematic surveys. We detected 51 L4 Trojans and 62 L5 Trojans ranging from 0.7 km to 13 km in diameter (D) (assuming an albedo of 0.04). We found that there is a difference of the cumulative size distribution between the L4 and L5 populations. The slopes of the cumulative size distribution of the L4 population with 2 km<D< 5 km and 5 km<D< 10 km were 1.3˙0.1 and 2.4 ˙0.1, respectively; meanwhile, that of the L5 population with 2 km&...
International audienceKnowing the shape distribution of an asteroid population gives clues to its co...
The Sub-Kilometer Asteroid Diameter Survey (SKADS) (Gladman et al. 2009) acquired good-quality orbit...
Context. A considerable amount of photometric data is produced by surveys such as Pan-STARRS, LONEOS...
We examined the size distributions of small L4 and L5 Jovian Trojan asteroids detected in the Subaru...
The importance of sub-kilometer-sized objects among the main-belt asteroids (MBAs) has been progress...
We present the results of a project to detect small (1 km) main-belt asteroids with the 3.6 m Canada...
Accepted for publication in Icarus - 43 pages, 15 figures, 7 tablesThe distribution of asteroids acr...
Aims. In this paper, we analyze the collisional and dynamical evolution of the population of L4 Jovi...
Aims.In this work we study the cumulative size distribution of the population of asteroids in come...
International audienceThe distribution of asteroids across the Main Belt has been studied for decade...
The Spitzer Asteroid Catalog contains flux measurements of asteroidsserendipitously observed in publ...
This thesis reports on new results on Trojan asteroids throughout the Solar System. Trojan asteroids...
Jupiter Trojan asteroid dynamics have been studied for a long time but it is only within the last de...
We present thermal observations of 44 Jovian Trojan asteroids with diameters D ranging from 5 to 24 ...
We present an analysis of survey observations targeting the leading L4 Jupiter Trojan cloud near opp...
International audienceKnowing the shape distribution of an asteroid population gives clues to its co...
The Sub-Kilometer Asteroid Diameter Survey (SKADS) (Gladman et al. 2009) acquired good-quality orbit...
Context. A considerable amount of photometric data is produced by surveys such as Pan-STARRS, LONEOS...
We examined the size distributions of small L4 and L5 Jovian Trojan asteroids detected in the Subaru...
The importance of sub-kilometer-sized objects among the main-belt asteroids (MBAs) has been progress...
We present the results of a project to detect small (1 km) main-belt asteroids with the 3.6 m Canada...
Accepted for publication in Icarus - 43 pages, 15 figures, 7 tablesThe distribution of asteroids acr...
Aims. In this paper, we analyze the collisional and dynamical evolution of the population of L4 Jovi...
Aims.In this work we study the cumulative size distribution of the population of asteroids in come...
International audienceThe distribution of asteroids across the Main Belt has been studied for decade...
The Spitzer Asteroid Catalog contains flux measurements of asteroidsserendipitously observed in publ...
This thesis reports on new results on Trojan asteroids throughout the Solar System. Trojan asteroids...
Jupiter Trojan asteroid dynamics have been studied for a long time but it is only within the last de...
We present thermal observations of 44 Jovian Trojan asteroids with diameters D ranging from 5 to 24 ...
We present an analysis of survey observations targeting the leading L4 Jupiter Trojan cloud near opp...
International audienceKnowing the shape distribution of an asteroid population gives clues to its co...
The Sub-Kilometer Asteroid Diameter Survey (SKADS) (Gladman et al. 2009) acquired good-quality orbit...
Context. A considerable amount of photometric data is produced by surveys such as Pan-STARRS, LONEOS...